Table A.1
Details of the spectroscopic HARPS-N observations presented in this work.
| Object | Type | Datea | UT Start | UT End | Nobs | Texp[s] | Airmassb | Moonc | 2nd fibre |
|---|---|---|---|---|---|---|---|---|---|
| HAT-P-3 | K5 | 2013.06.10 | 20:58 | 01:03 | 22 | 600 | 1.07 → 1.06 → 1.38 | NO | ThAr lamp |
| WASP-60 | F9d | 2013.10.20 | 21:08 | 02:59 | 21 | 900 | 1.07 → 1.00 → 1.59 | 95%/49° | Sky |
| HAT-P-22 | G2 | 2014.04.03 | 22:25 | 03:47 | 31 | 600 | 1.06 → 1.07 → 1.96 | NO | ThAr lamp |
| HAT-P-12 | K5 | 2015.03.13 | 00:59 | 06:22 | 21(17) | 900 | 1.20 → 1.03 → 1.22 | 46%/81° | Sky |
| 2015.04.24 | 20:56 | 01:02 | 16 | 900 | 1.48 → 1.03 | 41%/82° | Sky | ||
| WASP-39 | K5 | 2015.05.04 | 22:54 | 04:02 | 20 | 900 | 1.32 → 1.18 → 1.79 | 99%/ |
Sky |
Notes. (a) Dates refer to the beginning of the night. (b)Values at first → last exposure, or first → meridian → last exposure. (c)Fraction of illumination and angular distance from the target. (d)This work. (e)We checked that the nearby full Moon (RV = −3.5 km s−1) did not contaminate the CCF profiles and had no effect on the RV measurements (see Esposito et al. 2017).
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